Fig. A.1.
Comparison of mass accretion rate Ṁacc, mass loss rate of the O star Ṁwind, and Eddington accretion rate of the BH ṀEdd during the BH+O binary phase modelled from the 17 observed progenitor WR+O binaries for (β,η,γ±) = (0.8,1/3,1). The upper and lower panels present Ṁacc/Ṁwind and Ṁacc/ṀEdd, respectively. The colour coding in the legend denotes the 17 WR+O systems that are expected to form BH+O binaries.
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